18204Zeuthenfalse[["minutes", "Minutes"], ["notes", "Notes"], ["paper", "Paper"], ["poster", "Poster"], ["slides", "Slides"], ["summary", "Summary"]]Desy Zeuthenb12e9e859ad6be375e54cb3c3bd6fff710537tevpa2018@desy.deTeVPA 2018We are pleased to announce that the 2018 TeV Particle Astrophysics conference (TeVPA 2018) will take place in Berlin, Germany. TeVPA is a five day conference which aims to bring together leading scientists in the field to discuss recent advances in Astroparticle Physics.<br />
There is the possibility to host small workshops before and after the conference at DESY in Zeuthen (<a href="http://www.desy.de/about_desy/getting_there/zeuthen/index_eng.html" target="_blank">link</a>, ~50 km south of Berlin). In case of interest in this, please contact us at <a href="mailto:tevpa2018@desy.de">tevpa2018@desy.de</a>&nbsp;with a brief description of the workshop you would like to organize.FalseLVH, Luisenstraße 58, 10117 Berlin<a href="http://www.langenbeck-virchow-haus.de/" target="_blank"><b>LANGENBECK VIRCHOW HAUS</b></a>
Luisenstraße 58, 10117 Berlin2018-08-27T07:30:002018-08-31T17:25:002017-06-23T13:09:032018-11-26T08:40:56Europe/Berlin158false[["minutes", "Minutes"], ["notes", "Notes"], ["paper", "Paper"], ["poster", "Poster"], ["slides", "Slides"], ["summary", "Summary"]]DM09Dark Matter1Poster (A0 portrait)Constraints on MeV dark matter using neutrino detectors and their implication for the 21-cm resultsMs.GRAPPA institute, University of Amsterdameb7f20f1b0ff80eefba67d66d0e3aab2Ms.GRAPPA institute, University of Amsterdameb7f20f1b0ff80eefba67d66d0e3aab2University of Amsterdam157e18a9443ab70542022e368186296eLVH, Luisenstraße 58, 10117 Berlin<a href="http://www.langenbeck-virchow-haus.de/" target="_blank"><b>LANGENBECK VIRCHOW HAUS</b></a>
Luisenstraße 58, 10117 Berlin2018-08-28T15:45:002018-08-28T16:05:0000:20The recent results of the EDGES collaboration indicate that during the era of reionization, the primordial gas was much colder than expected. The cooling of the gas could be explained by interactions between dark matter (DM) and particles in the primordial gas. Constraints from cosmology and particle experiments indicate that this DM should be light (~10-80 MeV), mili-charged, and only make up a small fraction of the total amount of DM. Several constraints on the DM parameter space have already been made. We explore the still unconstrained space in the case that the mili-charged DM makes up for ~1% of the total DM, through the scenario in which this DM annihilates only into muon- and tau neutrinos. We set upper limits on the annihilation cross section using Super-Kamiokande data, and predict the upper limit that could be reached by future experiments like Hyper-Kamiokande. We show that these experiments might be able to reach the relevant parameter space predicted by EDGES, and therefore be capable to probe this DM scenario.